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Fig. 7


Mean neutron capture element abundances to the exclusion of the CH star, the CEMP-s star, and the metal-rich giant. The errorbars represent the star-to-star scatter. Also shown are the Solar r- and s-process contributions from Simmerer et al. (2004). Grey-shaded areas indicate the 1σ abundance ranges of the weak-r-process star HD 122563 from Honda et al. (2006). All curves were normalised to Eu.

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